The Solar Stellar Irradiance Comparison Experiment (SOLSTICE) is one of ten
instruments on the Upper Atmosphere Research Satellite (UARS) - one of two
instruments measuring the solar ultraviolet irradiance. The instrument is
a three channel spectrometer covering the spectral range 120 to 420 nm with
a spectral resolution of approximately 0.2 nm. It has been successfully op
erating since October 1991, and has now provided more than eight years of d
ata, extending from near the peak of solar cycle 22, through solar minimum
and into the new cycle. The data provide time series that display solar var
iations over time scales from a few days up to the 11-year solar cycle. Qua
ntitative estimates of amplitudes of both rotational modulation and the sol
ar cycle variation in the 1991-1999 epoch are given for the UV spectrum bet
ween 119 and 300 nm.